Do Indian economic activities impact ASEAN-5 stock markets?

This study examines the dynamic linkages of ASEAN-5 with India based on a multivariate framework. DCC-MGARCH model was used to assess the presence of contagion effects and herding behaviour, indicated by the dynamic conditional correlations. The var -Granger causality test was employed to capture the direction of dynamic volatility transmission at the short run. Findings showed that the dynamic correlation of ASEAN-5 stock markets with Indian economy is in par with the U.S. and Japan. The simultaneous sudden spike in Dynamic Conditional Correlation between India and ASEAN-5 and followed by immediate reversal to decreasing Dynamic Conditional Correlation in 2009 indicate a contagion effect and herding behaviour which coincided with European sovereign debt crisis. The immediate reversal back to decreasing Dynamic Conditional Correlation suggests that both countries are hardly contagious by external crisis. In the short run, there is no volatility spillover from Indian economic activities to ASEAN-5 stock markets but there is volatility spillover from stock markets of Indonesia and Singapore to Indian economic activities. Trade policies, economic crises and economic liberalisation play significant roles in shaping the structure of the dynamic volatility correlations between the studied markets. This study reveals that ASEAN-5 has become preferred markets for the diversification of stock portfolio for India in the short run

Recipes for Men: Manufacturing Make-up and the Politics of Production in 1910s China

In the first decade of Republican China (1911–49), masculinity was explored in writings on how to manufacture makeup that appeared in women’s magazines. Male authors and editors of these writings—some of whom were connoisseurs of technology, some of whom were would-be manufacturers—appropriated the tropes of the domestic and feminine to elevate hands-on work and explore industry and manufacturing as legitimate masculine pursuits. Tapping into time-honored discourses of virtuous productivity in the inner chambers and employing practices of appropriating the woman’s voice to promote unorthodox sentiment, these recipes “feminized” production to valorize a new masculine agenda, which included chemistry and manufacturing, for building a new China

Surveillance of colonization and infection with Staphylococcus aureus susceptible or resistant to methicillin in a community skilled-nursing facility

Background: Methicillin-resistant Staphylococcus aureus (MRSA) is an important nosocomial pathogen in acute care hospitals and long-term care facilities. Few studies have been reported in private skilled nursing facilities (SNFs) not experiencing outbreaks of infections caused by MRSA. METHODS: From a 149-bed SNF with no outbreaks, we report a 1-year prospective surveillance study of S. aureus colonization and infection, with focus on S. aureus phenotypes, both methicillin susceptible (MS) and methicillin resistant (MR). Nasal and stool or rectal screening cultures were done on admission, and all patients underwent screening on at least a quarterly basis for 1 year. RESULTS: Overall, 35% of patients were colonized at least once with S. aureus, (72% MS, 25% MR, and 3% mixed phenotypes), 94% of the MRSA were ciprofloxacin resistant. Nasal colonization with any S. aureus was more frequent, but 13% of patients had positive results only in rectal specimens. Twenty-one percent of the newly admitted and 15% of continuing patients acquired colonization during their stay in the SNE Colonization was transient or persistent, persisted longer in the nares compared with colonization in rectal specimens, and was more stable for methicillin-susceptible S. aureus. Nine percent of patients had development of infection with S. aureus. There was no indication that MRSA colonization led to more infections than methicillin-susceptible S. aureus. Of the 13 infected patients in whom cultures had previously been obtained, seven (54%) had been colonized by the same phenotype strains. CONCLUSIONS: In this private SNF, endemic S. aureus infections occur at a low frequency, reflecting a moderate level of colonization with S. aureus. However, a trend showing gradual increases in frequencies of colonization and infection is of concern and suggests that in this SNF, future intervention could become warranted

Introduction: The Entangled Histories of Science and Capitalism

This volume revisits the mutually constitutive relationship between science and capitalism from the seventeenth century to the present day. Adopting a global approach, this introduction rejects the notion that either science or capitalism can be understood as stages of modernity that emerged in the West and subsequently engendered a “Great Divergence” with the rest of the world. Instead, both science and capitalism were historical institutions that arose in an imperial context of global exchange and whose entanglement has been continuously remade. Rather than seek to explain either the development of modern science as a product of economic forces or the divergence of capitalist economies as a result of technical innovation, we want to emphasize the knowledge work that has been a central feature of both modern science and capitalism across the globe

Extreme Ultra-Violet Spectroscopy of the Lower Solar Atmosphere During Solar Flares

The extreme ultraviolet portion of the solar spectrum contains a wealth of diagnostic tools for probing the lower solar atmosphere in response to an injection of energy, particularly during the impulsive phase of solar flares. These include temperature and density sensitive line ratios, Doppler shifted emission lines and nonthermal broadening, abundance measurements, differential emission measure profiles, and continuum temperatures and energetics, among others. In this paper I shall review some of the advances made in recent years using these techniques, focusing primarily on studies that have utilized data from Hinode/EIS and SDO/EVE, while also providing some historical background and a summary of future spectroscopic instrumentation.Comment: 34 pages, 8 figures. Submitted to Solar Physics as part of the Topical Issue on Solar and Stellar Flare

Solar irradiance variability: a six-year comparison between SORCE observations and the SATIRE model

Aims: We investigate how well modeled solar irradiances agree with measurements from the SORCE satellite, both for total solar irradiance and broken down into spectral regions on timescales of several years. Methods: We use the SATIRE model and compare modeled total solar irradiance (TSI) with TSI measurements between 2003 and 2009. Spectral solar irradiance over 200-1630nm is compared with the SIM instrument on SORCE between 2004 and 2009 during a period of decline from moderate activity to the recent solar minimum in 10 nm bands and for three spectral regions of significant interest: the UV integrated over 200-300nm, the visible over 400-691nm and the IR between 972-1630 nm. Results: The model captures 97% of observed TSI variation. In the spectral comparison, rotational variability is well reproduced, especially between 400 and 1200 nm. The magnitude of change in the long-term trends is many times larger in SIM at almost all wavelengths while trends in SIM oppose SATIRE in the visible between 500 and 700nm and between 1000 and 1200nm. We discuss the remaining issues with both SIM data and the identified limits of the model, particularly with the way facular contributions are dealt with, the limit of flux identification in MDI magnetograms during solar minimum and the model atmospheres in the IR employed by SATIRE. It is unlikely that improvements in these areas will significantly enhance the agreement in the long-term trends. This disagreement implies that some mechanism other than surface magnetism is causing SSI variations, in particular between 2004 and 2006, if the SIM data are correct. Since SATIRE was able to reproduce UV irradiance between 1991 and 2002 from UARS, either the solar mechanism for SSI variation fundamentally changed around the peak of cycle 23, or there is an inconsistency between UARS and SORCE UV measurements. We favour the second explanation.Comment: 14 pages, 13 figure

Percentile reference values for anthropometric body composition indices in European children from the IDEFICS study

INTRODUCTION: To characterise the nutritional status in children with obesity or wasting conditions, European anthropometric reference values for body composition measures beyond the body mass index (BMI) are needed. Differentiated assessment of body composition in children has long been hampered by the lack of appropriate references. OBJECTIVES: The aim of our study is to provide percentiles for body composition indices in normal weight European children, based on the IDEFICS cohort (Identification and prevention of Dietary-and lifestyle-induced health Effects in Children and infantS). METHODS: Overall 18 745 2.0-10.9-year-old children from eight countries participated in the study. Children classified as overweight/obese or underweight according to IOTF (N = 5915) were excluded from the analysis. Anthropometric measurements (BMI (N = 12 830); triceps, subscapular, fat mass and fat mass index (N = 11 845-11 901); biceps, suprailiac skinfolds, sum of skinfolds calculated from skinfold thicknesses (N = 8129-8205), neck circumference (N = 12 241); waist circumference and waist-to-height ratio (N = 12 381)) were analysed stratified by sex and smoothed 1st, 3rd, 10th, 25th, 50th, 75th, 90th, 97th and 99th percentile curves were calculated using GAMLSS. RESULTS: Percentile values of the most important anthropometric measures related to the degree of adiposity are depicted for European girls and boys. Age-and sex-specific differences were investigated for all measures. As an example, the 50th and 99th percentile values of waist circumference ranged from 50.7-59.2 cm and from 51.3-58.7 cm in 4.5-to < 5.0-year-old girls and boys, respectively, to 60.6-74.5 cm in girls and to 59.9-76.7 cm in boys at the age of 10.5-10.9 years. CONCLUSION: The presented percentile curves may aid a differentiated assessment of total and abdominal adiposity in European children

Derecho y Sociedad.

El derecho es un fenómeno social. Creación propia de la, sociedad, que lo forja y lo impone para su garantía y salvaguarda, varía con ella en función de tres factores: a) tiempo, b) espacio, y c) psicología del grupo

Derecho y Sociedad.

El derecho es un fenómeno social. Creación propia de la, sociedad, que lo forja y lo impone para su garantía y salvaguarda, varía con ella en función de tres factores: a) tiempo, b) espacio, y c) psicología del grupo

Variability of Sun-like stars: reproducing observed photometric trends

The Sun and stars with low magnetic activity levels, become photometrically brighter when their activity increases. Magnetically more active stars display the opposite behaviour and get fainter when their activity increases. We reproduce the observed photometric trends in stellar variations with a model that treats stars as hypothetical Suns with coverage by magnetic features different from that of the Sun. The presented model attributes the variability of stellar spectra to the imbalance between the contributions from different components of the solar atmosphere, such as dark starspots and bright faculae. A stellar spectrum is calculated from spectra of the individual components, by weighting them with corresponding disc area coverages. The latter are obtained by extrapolating the solar dependences of spot and facular disc area coverages on chromospheric activity to stars with different levels of mean chromospheric activity. We have found that the contribution by starspots to the variability increases faster with chromospheric activity than the facular contribution. This causes the transition from faculae-dominated variability and direct activity--brightness correlation to spot-dominated variability and inverse activity--brightness correlation with increasing chromospheric activity level. We have shown that the regime of the variability also depends on the angle between the stellar rotation axis and the line-of-sight and on the latitudinal distribution of active regions on the stellar surface. Our model can be used as a tool to extrapolate the observed photometric variability of the Sun to Sun-like stars at different activity levels, which makes possible the direct comparison between solar and stellar irradiance data.Comment: 20 pages, 16 figures, accepted for publication in Astronomy&Astrophysic